Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1409.6724.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T22:18:28.282576Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
77
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation c37ecebd-189f-4657-a258-062fa5b92f44 · inbound
Abundant Water from Early Supernovae at Cosmic Dawn cites this paper.
Abundant Water from Early Supernovae at Cosmic Dawn CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:18:28.282576Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e743ef67-e68a-4b0f-8c5e-696c6a4e7493 · inbound
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity
Reference 99
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T04:20:32.341773Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 3b1b39dc-7090-43a4-957e-5ae79aba1ae7 · inbound
End-to-end differentiable retrieval of molecular spectra using hydrodynamics, chemistry, and radiative transfer cites this paper.
End-to-end differentiable retrieval of molecular spectra using hydrodynamics, chemistry, and radiative transfer CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity
Reference 206
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T00:39:21.815543Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.